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Black holes quasinormal modes, Loop Quantum Gravity Immirzi parameter and nonextensive statistics.
- Source :
-
Physics Letters B . Nov2019, Vol. 798, pN.PAG-N.PAG. 1p. - Publication Year :
- 2019
-
Abstract
- It is argued that, using the black hole area entropy law together with the Boltzmann-Gibbs statistical mechanics and the quasinormal modes of the black holes, it is possible to determine univocally the lowest possible value for the spin j in the context of the Loop Quantum Gravity theory which is j m i n = 1. Consequently, the value of Immirzi parameter is given by γ = ln 3 / (2 π 2). In this paper, we have shown that if we use Tsallis microcanonical entropy rather than Boltzmann-Gibbs framework then the minimum value of the label j depends on the nonextensive q -parameter and may have values other than j m i n = 1. [ABSTRACT FROM AUTHOR]
Details
- Language :
- English
- ISSN :
- 03702693
- Volume :
- 798
- Database :
- Academic Search Index
- Journal :
- Physics Letters B
- Publication Type :
- Academic Journal
- Accession number :
- 139408037
- Full Text :
- https://doi.org/10.1016/j.physletb.2019.135011